5XMM J105241.5+573650
5XMM-DR15 stacked source · SRCID 3002274010100024
Position:
10h52m41.52s +57d36m50.6s
(163.17300°, 57.61406°)
EP flux
4.14e-14
± 2.0e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.764)
Detections
16
| SRCID | 3002274010100024 |
|---|---|
| IAUNAME | 5XMM J105241.5+573650 |
| SC_RA | 10h52m41.52s (163.17300°) |
| SC_DEC | +57d36m50.6s (57.61406°) |
| RADEC_ERR | 0.13 arcsec |
| LII / BII | 149.1199° / 53.0526° |
| N_CONTRIB | 16 (detections) |
| N_OBS | 21 (observations covering the position) |
| MJD_FIRST | 51661.158 (2000-04-27 03:47:47.000 UTC) |
| MJD_LAST | 52615.196 (2002-12-07 04:41:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.14e-14 ± 2.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.33
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.37
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.16
± 0.02
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44
± 0.04
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.4)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 0.961
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
Optical Monitor (OM)
- OM Source ID
- 2957853
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.266 | 0.073 |
| U | 21.593 | 0.038 |
| B | 20.173 | 0.029 |
| V | 19.082 | 0.045 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.08e-14 (+6.5e-14 / −5.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.20e+20 (+1.1e+21 / −3.6e+20) cm−2 |
| Photon index (Γ) | 1.42 (+1.53 / −1.29) |
| DoF | 788 |
| p-value | 0.67 |
| Inter-instrument norm. | 0.99 (0.91–1.07) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 11.500 (approximate flux variability amplitude) |
|---|
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.